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dc.contributor.authorBilir, Selçuk
dc.contributor.authorAk, S.
dc.contributor.authorAk, Tansel
dc.contributor.authorRETTER, A.
dc.date.accessioned2021-03-04T19:41:47Z
dc.date.available2021-03-04T19:41:47Z
dc.date.issued2007
dc.identifier.citationAk T., Bilir S., Ak S., RETTER A., "A new absolute magnitude calibration with 2MASS for cataclysmic variables", NEW ASTRONOMY, cilt.12, ss.446-453, 2007
dc.identifier.issn1384-1076
dc.identifier.otherav_91052dc2-3f7a-4356-bbbb-26f40bd3b0ef
dc.identifier.othervv_1032021
dc.identifier.urihttp://hdl.handle.net/20.500.12627/97850
dc.identifier.urihttps://doi.org/10.1016/j.newast.2007.01.002
dc.description.abstractUsing reliable trigonometric measurements, we find that the absolute magnitude of cataclysmic variables depends on the orbital period and de-reddened (J - H)(0) and (H - K-s)(0) colours of 2MASS (Two Micron All Sky Survey) photometric system. The calibration equation covers the ranges 0.032(d) < P-orb <= 0.454(d) , -0.08 < (J - H)(0) <= 1.54, -0.03 < (H - K-s)(0) <= 0.56 and 2.0 <= M-J < 11.7; It is based on trigonometric parallaxes with relative errors of (sigma(pi)/pi) <= 0.4. By using the period-1 uminosity-colours (PLCs) relation, we estimated the distances of cataclysmic variables with orbital periods and 2MASS observations and compared them with distances found from other methods. We suggest that the PLCs relation can be a useful statistical tool to estimate the distances of cataclysmic variables. (C) 2007 Elsevier B.V. All rights reserved.
dc.language.isoeng
dc.subjectFizik
dc.subjectASTRONOMİ VE ASTROFİZİK
dc.subjectUzay bilimi
dc.subjectTemel Bilimler (SCI)
dc.subjectAstronomi ve Astrofizik
dc.subjectTemel Bilimler
dc.titleA new absolute magnitude calibration with 2MASS for cataclysmic variables
dc.typeMakale
dc.relation.journalNEW ASTRONOMY
dc.contributor.department, ,
dc.identifier.volume12
dc.identifier.issue6
dc.identifier.startpage446
dc.identifier.endpage453
dc.contributor.firstauthorID53893


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